A High-Temperature Al–Ca Condensate in the Lunar Regolith


Cite item

Full Text

Open Access Open Access
Restricted Access Access granted
Restricted Access Subscription Access

Abstract

For the first time, a high-temperature condensate in the form of two-component glass beads of about 200–400 nm size, consisting of an Al–Ca oxide core rimmed by a uniform oxide film of high-silica glass containing iron nano-inclusions, has been found in natural samples of the lunar regolith from Mare Crisium (Luna-24). Earlier, a high-temperature condensate was only theoretically predicted on the basis of laser evaporation experiments.

About the authors

A. V. Mokhov

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences (IGEM RAS)

Author for correspondence.
Email: avm8okhov@gmail.com
Russian Federation, Moscow, 119017

T. A. Gornostaeva

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences (IGEM RAS)

Email: avm8okhov@gmail.com
Russian Federation, Moscow, 119017

P. M. Kartashov

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences (IGEM RAS)

Email: avm8okhov@gmail.com
Russian Federation, Moscow, 119017

A. P. Rybchuk

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences (IGEM RAS)

Email: avm8okhov@gmail.com
Russian Federation, Moscow, 119017

O. A. Bogatikov

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences (IGEM RAS)

Email: avm8okhov@gmail.com
Russian Federation, Moscow, 119017


Copyright (c) 2019 Pleiades Publishing, Ltd.

This website uses cookies

You consent to our cookies if you continue to use our website.

About Cookies